The LSPE-Strip feed horn array

Journal of Instrumentation IOP Publishing 17:01 (2022) p01029

Authors:

C Franceschet, F Del Torto, F Villa, S Realini, R Bongiolatti, OA Peverini, F Pezzotta, DM Viganó, G Addamo, M Bersanelli, F Cavaliere, F Cuttaia, M Gervasi, A Mennella, G Morgante, AC Taylor, G Virone, M Zannoni

The large scale polarization explorer (LSPE) for CMB measurements: performance forecast

Journal of Cosmology and Astroparticle Physics IOP Publishing 2021:08 (2021) 008

Authors:

G Addamo, PAR Ade, C Baccigalupi, AM Baldini, PM Battaglia, ES Battistelli, A Baù, P de Bernardis, M Bersanelli, M Biasotti, A Boscaleri, B Caccianiga, S Caprioli, F Cavaliere, F Cei, KA Cleary, F Columbro, G Coppi, A Coppolecchia, F Cuttaia, G D'Alessandro, G De Gasperis, M De Petris, V Fafone, F Farsian, L Ferrari Barusso, F Fontanelli, C Franceschet, TC Gaier, L Galli, F Gatti, R Genova-Santos, M Gerbino, M Gervasi, T Ghigna, D Grosso, A Gruppuso, R Gualtieri, F Incardona, ME Jones, P Kangaslahti, N Krachmalnicoff, L Lamagna, M Lattanzi, CH López-Caraballo, M Lumia, R Mainini, D Maino, S Mandelli, M Maris, S Masi, S Matarrese, A May, L Mele, P Mena, A Mennella, R Molina, D Molinari, G Morgante, U Natale, F Nati, P Natoli, L Pagano, A Paiella, F Panico, F Paonessa, S Paradiso, A Passerini, M Perez-de-Taoro, OA Peverini, F Pezzotta, F Piacentini, L Piccirillo, G Pisano, G Polenta, D Poletti, G Presta, S Realini, N Reyes, A Rocchi, JA Rubino-Martin, M Sandri, S Sartor, A Schillaci, G Signorelli, B Siri, M Soria, F Spinella, V Tapia, A Tartari, AC Taylor, L Terenzi, M Tomasi, E Tommasi, C Tucker, D Vaccaro, DM Vigano, F Villa, G Virone, N Vittorio, A Volpe, REJ Watkins, A Zacchei, M Zannoni

The LSPE-Strip feed horn array

ArXiv 2107.13775 (2021)

Authors:

C Franceschet, F Del Torto, F Villa, S Realini, R Bongiolatti, OA Peverini, F Pezzotta, DM Viganó, G Addamo, M Bersanelli, F Cavaliere, F Cuttaia, M Gervasi, A Mennella, G Morgante, AC Taylor, G Virone, M Zannoni

MID-Radio Telescope, single pixel feed packages for the square kilometre array: an overview

IEEE Journal of Microwaves Institute of Electrical and Electronics Engineers 1:1 (2021) 428-437

Authors:

Angela Taylor, Michael Jones, Jamie Leech, andre Hector, Lei Liu, Robert Watkins, A Pellegrini

Abstract:

The Square Kilometre Array (SKA) project is an international effort to build the world’s largest radio telescope, enabling science with unprecedented detail and survey speed. The project spans over a decade and is now at a mature stage, ready to enter the construction and integration phase. In the fully deployed state, the MID-Telescope consists of a 150-km diameter array of offset Gregorian antennas installed in the radio quiet zone of the Karoo desert (South Africa). Each antenna is equipped with three feed packages, that are precision positioned in the sub-reflector focus by a feed indexer platform. The total observational bandwidth (0.35-15.4GHz) is segmented into seven bands. Band 1 (0.35 – 1.05 GHz) and Band 2 (0.95 – 1.76 GHz) are implemented as individual feed packages. The remaining five bands (Bands 3, 4, 5a, 5b, and 6) are combined in a single feed package. Initially only Band 5a (4.6 – 8.5 GHz) and Band 5b (8.3 – 15.4 GHz) will be installed. This paper provides an overview of recent progress on design, test and integration of each feed package as well as project and science goals, timeline and path to construction.

MID-Radio Telescope, Single Pixel Feed Packages for the Square Kilometre Array: An Overview

IEEE Journal of Microwaves Institute of Electrical and Electronics Engineers (2021)

Authors:

Alice Pellegrini, Jonas Flygare, Isak P Theron, Robert Lehmensiek, Adriaan Peens-Hough, Jamie Leech, Michael E Jones, Angela C Taylor, Robert EJ Watkins, Lei Liu, Andre Hector, Biao Du, Yang Wu

Abstract:

The Square Kilometre Array (SKA) project is an international effort to build the world s largest radio telescope, enabling science with unprecedented detail and survey speed. The project spans over a decade and is now at a mature stage, ready to enter the construction and integration phase. In the fully deployed state, the MID-Telescope consists of a 150-km diameter array of offset Gregorian antennas installed in the radio quiet zone of the Karoo desert (South Africa). Each antenna is equipped with three feed packages, that are precision positioned in the sub-reflector focus by a feed indexer platform. The total observational bandwidth (0.35-15.4GHz) is segmented into seven bands. Band 1 (0.35-1.05GHz) and Band 2 (0.95-1.76GHz) are implemented as individual feed packages. The remaining five bands (Bands 3, 4, 5a, 5b, and 6) are combined in a single feed package. Initially only Band 5a (4.6-8.5GHz) and Band 5b (8.3-15.4GHz) will be installed. This paper provides an overview of recent progress on design, test and integration of each feed package as well as project and science goals, timeline and path to construction.